0000000000626004

AUTHOR

Laurence Sabin

showing 2 related works from this author

First results of an Hα based search of classical Be stars in the Perseus Arm and beyond

2013

We investigate a region of the Galactic plane, between 120 <= l <= 140 and -1 <= b <= +4, and uncover a population of moderately reddened (E(B-V) \sim 1) classical Be stars within and beyond the Perseus and Outer Arms. 370 candidate emission line stars (13 <= r <= 16) selected from the INT Photometric H-alpha Survey of the Northern Galactic plane (IPHAS) have been followed up spectroscopically. A subset of these, 67 stars with properties consistent with those of classical Be stars, have been observed at sufficient spectral resolution (Delta_lambda \sim 2 - 4 Angstrom) at blue wavelengths to narrow down their spectral types. We determine these to a precision estimated to be…

PhysicsSpiral galaxyK-type main-sequence starExtinction (astronomy)Perseus ArmFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalactic planeStellar classificationAstrophysics - Astrophysics of GalaxiesStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsEquivalent widthSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
researchProduct

The second data release of the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS DR2)

2014

The INT/WFC Photometric H-Alpha Survey of the Northern Galactic Plane (IPHAS) is a 1800 square degrees imaging survey covering Galactic latitudes |b| < 5 deg and longitudes l = 30 to 215 deg in the r, i and H-alpha filters using the Wide Field Camera (WFC) on the 2.5-metre Isaac Newton Telescope (INT) in La Palma. We present the first quality-controlled and globally-calibrated source catalogue derived from the survey, providing single-epoch photometry for 219 million unique sources across 92% of the footprint. The observations were carried out between 2003 and 2012 at a median seeing of 1.1 arcsec (sampled at 0.33 arcsec/pixel) and to a mean 5\sigma-depth of 21.2 (r), 20.0 (i) and 20.3 (H-a…

InfraredAstronomyFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionRoot mean squarePhotometry (optics)surveyslaw0103 physical sciencesQB460stellar content [Galaxy]010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)cataloguesPhysics010308 nuclear & particles physicsNewtonian telescopeVegaAstronomyAstronomy and AstrophysicsBeGalactic planeemission-line [stars]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - Instrumentation and Methods for AstrophysicsData releaseData reduction
researchProduct